Thermochronological, petrographic and geochemical characteristics of the Combia Formation, Amagá basin, Colombia Matthias Bernet, Juliana Mesa Garcia, Catherine Chauvel, Maria Ramírez Londoño, Maria Marín-Cerón
To cite this version:
Matthias Bernet, Juliana Mesa Garcia, Catherine Chauvel, Maria Ramírez Londoño, Maria Marín- Cerón. Thermochronological, petrographic and geochemical characteristics of the Combia Forma- tion, Amagá basin, Colombia. Journal of South American Earth Sciences, Elsevier, 2020, 104, 10.1016/j.jsames.2020.102897. hal-02990433
HAL Id: hal-02990433 https://hal.archives-ouvertes.fr/hal-02990433 Submitted on 17 Nov 2020
HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. 1 Thermochronological, petrographic and geochemical 2 characteristics of the Combia Formation, Amagá basin, Colombia
3
4 Matthias Bernet1*, Juliana Mesa Garcia2,3, Catherine Chauvel1,4
5 and Maria Isabel Marín-Cerón2,
6 1Institut des Sciences de la Terre, CNRS, Université Grenoble Alpes, Grenoble, 7 France 8 2Departemento de Geociencias, Universidad EAFIT, Medellín, Colombia 9 10 3present address: Geology Department, University of Michigan, Ann Arbor, MI, USA 11 12 4Université de Paris, Institut de Physique du Globe de Paris, CNRS,F-75005 Paris, 13 France 14 15 *corresponding author, email: [email protected], 16 ORCID: 0000-0001-5046-7520 17
18
19 Abstract
20 The Amagá basin between the Western and Central Cordilleras of the
21 Northern Andes of Colombia host the Neogene volcanic and volcaniclastic Combia
22 Formation. At this stage it is not clear how the formation of this unit is related to arc
23 volcanism and which role the Nazca plate subduction beneath the western margin of
24 South America plays. The timing, petrography and geochemical characteristics of
25 Combia Formation rocks were studied in the western and eastern parts of the
26 Amagá basin, in order to gain more information on the type of magma generation
27 and volcanic activity that led to the deposition of the Combia Formation.
28 Apatite and zircon fission-track dating largely confirm a 12-6 Ma age for the
29 deposition of the Combia Formation. Petrographic and major element analyses show
30 that mainly trachy-andesite ignimbrites with a calc-alkaline composition were
31 deposited in the western Amagá basin, whereas the volcanic rocks of the eastern
1
32 Amagá basin are lava flow and fall-out deposits of basaltic andesites or of tholeiitic
33 composition. Trace element and isotopic analyses show that slab dehydration and
34 sediment melting were important in primary magma generation in the mantle wedge,
35 but the primary magma was mixed with lower continental crustal melts, resulting in
36 characteristic isotope signatures in the western and eastern Amagá basin. All this
37 points to subduction driven arc volcanism with slab dehydration, sediment melting
38 magma mixing.
39
40
41 Introduction
42 The late Paleogene to present-day magmatism of northwestern South
43 America can be divided into four major phases of activity at about 24-20 Ma, 12-6
44 Ma, 6-3 Ma, and 3 Ma to the Present (e.g. Sierra, 1994; Toro et al., 1999; Gonzalez,
45 2001; Ramírez et al., 2006; Cediel et al., 2011; Pérez et al., 2013; Lesage et al.,
46 2013). These different magmatic phases are related to the complex tectonic setting
47 in which the Caribbean, Nazca and South American plates interact with each other
48 (Fig. 1). The break-up of the Farallón plate into the Nazca and Cocos plates between
49 26 and 24 Ma (Marriner and Millward, 1984), the reorientation of subduction
50 direction (Pardo-Casas and Molnar, 1987), and collision of the Panamá-Choco block
51 with northwestern South America at about 25 Ma drove the first magmatic pulse (e.g.
52 McCourt et al., 1984; Aspden et al., 1987; Kellogg and Vega, 1995; Trenkamp et al.,
53 2002; Cediel et al., 2003; Lonsdale, 2005; Restrepo-Moreno et al., 2010; Farris et
54 al., 2011). Second, since the late Paleogene the Nazca plate subduction zone was
55 subjected to changes in subduction angle and direction over time, resulting in
56 Miocene-Pliocene magmatic intrusions in the Western and Central Cordillera and
2
57 deposition of the Combia Formation in the Amagá basin (e.g. Pardo-Casas and
58 Molnar, 1987; Taboada et al., 2000; Cediel et al., 2003; Vargas and Mann, 2013). At
59 the same time, subduction of the Caribbean plate beneath the northern (Caribbean)
60 margin of South America caused isolated late Miocene-Pliocene volcanic activity in
61 the Eastern Cordillera (e.g. Vargas and Mann, 2013), such as in the Vetas-California
62 gold-mining district of the Santander Massif (Mantilla et al., 2013), or the Paipa-Iza
63 complex 150 km to the north-east of Bogotá (Fig. 1; Padro et al., 2005; Bernet et al.,
64 2016). Today the main volcanic activity in Colombia is focused on the Central
65 Cordillera with for example the Nevado del Ruiz, Nevado del Tolima, Cerro Machín,
66 Nevado del Huila, Azufral, Cumbal, etc. well to the south of the study area (Fig. 1;
67 e.g. Marín-Cerón et al., 2010, 2019; Leal-Mejía, 2011).
68 Different techniques have been used for more than a century to understand
69 the genesis, age and evolution of the Combia Formation, including petrography,
70 heavy mineral analysis, X-ray diffraction, geochemistry, geochronology,
71 thermochronology and stratigraphic analyses (e.g. Grosse, 1926; Jaramillo, 1976;
72 Calle and González, 1980; Álvarez, 1983; Marriner and Millward, 1984; Rios and
73 Sierra, 2004; Pérez, 2005; López et al., 2006; Ramírez et al., 2006), but the
74 evolution of the Nazca plate subduction zone magmatism still remains poorly
75 constrained. Here we present a study of a suite of samples collected from three
76 sections, the Cerro Amarillo section in the eastern Amagá basin, and the Anzá-
77 Bolombolo and La Metida Creek sections in the western Amagá basin (Fig. 2), in
78 order to improve the knowledge gained so far about the Combia Formation. The
79 volcaniclastic, tuff/lapilli and flow deposits of the Combia Formation were examined
80 with a) apatite fission-track (AFT) and zircon fission-track (ZFT) thermochronology,
81 b) petrographic analyses, and c) major and trace element analysis, as well as Sr, Nd
3
82 and Pb isotope analyses. All this was done with the objective of a) characterizing
83 and comparing the eastern and western volcanic deposits, and b) to better
84 understand the mid-late Miocene evolution of the Nazca subduction zone
85 magmatism manifested between the Western and Central Cordilleras.
86
87 Geological setting
88 The Northern Andes of northwestern South America consist in Colombia of
89 the Western, Central and Eastern Cordilleras (Fig. 1). Each of these mountain belts
90 reflects a particular part of the long-term evolution of the Northern Andes, which is
91 characterized by magmatic episodes since the Precambrian, during the Triassic,
92 Jurassic, Late Cretaceous, and since the late Paleogene/Neogene until today
93 (Aspden et al., 1987). In general, these magmatic phases have been related to
94 Farallón/Nazca plate subduction beneath the western margin of the South American
95 plate (e.g. Marriner and Millward, 1984; McCourt et al., 1984; Cediel et al., 2003;
96 Saenz, 2003; Restrepo-Moreno et al., 2009; Rodríguez et al., 2012). Accretion of
97 tectonic blocks or terranes of oceanic affinity to the continental margin during the late
98 Mesozoic and early Cenozoic did not cause Andean-type subduction volcanism,
99 because of their relatively young age and high buoyancy preventing subduction
100 (Cediel et al., 2003), and forcing surface uplift and the formation of the Western and
101 Central Cordilleras during the Pre-Andean and Andean orogenies (e.g. Van der
102 Hammen, 1960; Taboada et al., 2000; Cediel et al., 2003).
103 The present-day Andean volcanism is commonly divided into four volcanic
104 zones, the Northern Volcanic Zone (NVZ), Central Volcanic Zone (CVZ), Southern
105 Volcanic Zone (SVZ), and Austral Volcanic Zone (AVZ) (e.g. Thorpe and Francis,
106 1979; Thorpe et al., 1982; Stern, 2004; Marín-Cerón et al., 2019). These segments
4
107 have been distinguished based on differences in petrographic features and
108 geochemical signatures, and they are separated from each other by volcanic gaps
109 (e.g. Thorpe and Francis, 1979; Stern, 2004). The NVZ is located in north-western
110 South America and encompasses the region of present-day volcanism in the
111 Northern Andes of Ecuador and Colombia.
112
113 Geology of the Amagá basin
114 The Amagá basin forms the northern part of the much larger Amagá-Cauca-
115 Patía basin located between the Western and Central Cordilleras of the Northern
116 Andes in western Colombia (Fig. 1; Sierra and Marín-Cerón, 2011). Dextral strike–
117 slip faulting along the Cauca and Romeral fault systems to the west and east
118 respectively is responsible for development of the Amagá basin, which is tectonically
119 a pull – apart basin (e.g. Cediel et al., 2003). Basin evolution started possibly during
120 the Eocene (?) – Oligocene, with surface uplift and erosion of the Central Cordillera
121 from the Late Cretaceous to Eocene and deposition of clastic sediments of the
122 Lower Amagá Formation in the basin (e.g. Restrepo-Moreno et al., 2009). The Lower
123 Amagá Formation is known for its quartz-rich sandstones and mainly sub-bituminous
124 but locally anthracite grade coal (Silva et al., 2008; Blandon et al., 2008). The Lower
125 Amagá Formation is separated from the Oligocene to Miocene Upper Amagá
126 Formation by an unconformity and a change to a lithic arenite composition with
127 sedimentary and metamorphic lithoclasts derived from the Central Cordillera (Paez
128 Acuna, 2012). During the mid to late Miocene, subduction of the Nazca plate below
129 the South American plate allowed the genesis of the Combia Formation in the
130 Amagá basin (e.g. Grosse, 1926; Marriner and Millward, 1984; González, 2001;
131 Cediel et al., 2003; Ramírez et al., 2006; Leal-Mejía, 2011; Cediel et al., 2011).
5
132 Therefore, the Upper Amagá Formation is overlain by volcanic and volcaniclastic
133 deposits of the Combia Formation. Here we focus on the Cerro Amarillo section in
134 the Eastern Amagá basin and the Anzá – Bolombolo and Le Metida Creek sections
135 in the western Amagá basin.
136
137 The Cerro Amarillo section
138 This section is located between the towns of Damasco and La Pintada (Fig.
139 2). It has a total thickness of 193 m and comprises 34 layers of welded tuff,
140 pyroclastic and agglomerate breccia, lapilli tuff breccia, basalt and scoria (Fig. 3).
141 The layers vary in thickness from a 20 m pyroclastic and agglomerate breccia to 0.3
142 m lapilli tuff breccia, both at the top (Mesa-Garcia, 2015). There is also a 19.2 m
143 thick welded tuff at the bottom. However, it is most common to find layers of 1 – 7 m
144 in thickness. The layers are characterized by a tabular geometry. No evidence of
145 pinchout or lenses were observed in the outcrops. The bottom of the stratigraphic
146 succession is mainly characterized by lava flows and welded tuff while, the top of the
147 sequence mainly consists in coarse to very coarse grained pyroclastic flows. The
148 bottom layers have a strike and dip of S05°E/25°SW in average; towards the middle
149 of the section the layers strike and dip N70°E/18°SE. Finally the top breccia and
150 lapilli tuff layers strike and dip N15°W/19SW. Many basalt and welded tuffs layers
151 have randomly distributed vesicles and amygdules of variable size shapes, some are
152 elongated indicating lava flow directions.
153
154 The Anzá – Bolombolo section
155 This section is also located on the western bank of the Cauca River (Fig. 2)
156 between the villages of Anzá and Bolombolo. The stratigraphy of the 11.04 m thick
6
157 succession consists of tuffs and lapilli tuffs in the lower part of the section, which are
158 separated laterally from andesitic basalts and ash flow deposits by an erosional
159 unconformity (Fig. 4; Grosse, 1926; González, 2001; Sierra and Marín-Cerón, 2011).
160 In the upper part of the succession are a lapilli tuff breccia and a non-differentiated
161 lava flow, which cover the underlying units and the unconformity. No particular
162 sedimentary structures were observed at this location.
163
164 The La Metida Creek section
165 This section is located on the western bank of the Cauca River to the west of
166 Bolombolo (Fig. 2). The Combia Formation crops out along the stream bed (e.g.
167 González, 2001) and the exposed stratigraphic sequence has a thickness of 45 m
168 and is composed of 33 layers of tuff, lapilli tuff, lapilli tuff breccia, pyroclastic flows
169 and volcano-clastic sandstones (Fig. 5). Sedimentary structures found throughout
170 the sequence include lenticular bedding, load structures, ripple lamination and cross-
171 bedding. The layers at the bottom are mainly grain-supported, whereas the top
172 layers are matrix-supported. In addition, nodules and organic matter are commonly
173 observed at the bottom of the section, and the middle section is characterized by
174 bioturbation and fossilized plants (e.g. leaves). No such material was observed
175 towards the top of the section.
176
177 Analytical methods
178 Apatite and zircon fission-track analyses
179 AFT analysis was done on two samples from the AB section and six samples
180 from the MC section. In addition, ten samples of the MC section were analyzed with
7
181 the ZFT method. Unfortunately, the apatite and zircon yield of the CA section
182 samples was too low for fission-track analyses.
183 Sample preparation and analyses were performed at the thermochronology
184 laboratory of the Universidad EAFIT at Medellín and the ISTerre thermochronology
185 laboratory at the Université Grenoble Alpes. Rock samples were crushed and sieved
186 and heavy mineral fractions were separated using standard hydraulic, magnetic and
187 heavy liquid separation techniques. The apatite crystals were mounted in epoxy and
188 the zircon crystals in Teflon® sheets, polished and etched. Apatite grains were
189 etched for 20 seconds at 21°C with 5.5 mol HNO3, and zircons were etched at 228°C
190 for 10-40 h in a NaOH-KOH melt to reveal fission tracks. A white mica sheet was
191 mounted as the external detector. All samples were irradiated with thermal neutrons
192 at the FRM II reactor in Garching, Germany, with a nominal fluence of 8x1015 n/cm2
193 for apatite and 0.5x1015 n/cm2 for zircon, together with IRMM540R dosimeter glasses
194 and Durango age standards for apatite, and IRMM541 dosimeter glasses and Buluk
195 and Fish Canyon Tuff age standards for zircon. After irradiation external detectors
196 were etched in 48% HF for 18 min at 21°C. Fission tracks were counted dry at 1250x
197 using an Olympus BX51 microscope and the FTStage 4.04 system. Fission-track
198 ages for each sample were calculated using the Binomfit software of Brandon (see
199 Ehlers et al., 2005) and the RadialPlotter program of Vermeesch (2009).
200
201 Petrographic analyses
202 Petrographic analyses were performed on twenty samples, seven from the
203 Cerro Amarillo section, three from the Anzá-Bolombolo section, and ten from the La
204 Metida Creek section. Petrographic thin sections were prepared at Geoensayos
8
205 S.A.S., Medellín, Colombia. Some of the pyroclastic samples had to be impregnated
206 with epoxy, as these deposits were not well consolidated.
207 The samples were analyzed using an Olympus BX41TF petrographic
208 microscope at the Geology department of EAFIT University. Modal analysis was
209 performed counting 300 – 500 points per sample, using a point counter. The
210 description of mineral assemblages and textures was done according to Mackenzie
211 et al. (1984) and Ehlers (1987). The samples were classified using modal mineral
212 composition and the QAP diagram of Streckeisen (1976) for volcanic rocks and
213 based on the size of the material after Pettijohn (1975) for pyroclastic rocks.
214
215 Geochemical analyses
216 The rock samples collected in the field were crushed to 1 mm chips at the
217 Laboratory of Solid Materials at EAFIT University. Two hundred grams per sample
218 were separated thoroughly, choosing the rock chips that were the least weathered
219 and geochemical analyses for major and trace elements were performed in the clean
220 laboratory at the Institut des Sciences de la Terre (ISTerre) – Université Grenoble
221 Alpes, France. Samples were finely powdered in an agate mortar previous to
222 analyses, except for Pb isotope analysis for which rock chips were used directly. The
223 sample preparation and analytical procedures were executed according to Chauvel
224 et al. (2011), as summarized below.
225 For major elements, 50 mg of powdered sample were dissolved in 800 µl of
226 concentrated HNO3 and 15 drops of concentrated HF and heated in a Savillex
227 beaker for two days at 90°C on a hot plate. After cooling, 20 ml of H3BO3 (25 g/l)
228 were added to the solution to neutralize excess HF, 10 g of HNO3 and 250 ml of
229 milliQ water for further dilution. Five standards (BR 24, BEN, BHVO2, AGV–1 and
9
230 BCR–1), a duplicate and a blank were as well prepared for analysis. The solutions
231 were analyzed using Inductively Coupled Plasma Atomic Emission Spectroscopy
232 (ICP AES) at ISTerre to determine the major element composition of each sample.
233 Concentrations were obtained using the international rock standard BR to calibrate
234 the signal and the values recommended by Chauvel et al. (2011). Loss on ignition
235 (LOI) was calculated for all samples by heating one gram of sample at 1000°C for
236 one hour.
237 Sixteen samples, five standards (BR 24, BEN, BHVO2, AGV–1 and BCR–1),
238 three duplicates and one blank were analyzed for trace element contents. One
239 hundred milligrams of samples and standards were dissolved in 20 drops of
240 concentrated HNO3 and 3 ml of HF for three days at 120°C in Savillex beakers.
241 Samples were further taken up in 7N HNO3 and finally dissolved in 2% HNO3 with
242 traces of HF, to obtain a dilution factor of about 5000 (Chauvel et al., 2011). The
243 sample was analyzed using an Inductively Coupled Plasma Mass Spectrometry (ICP
244 MS) Agilent 7500 at ISTerre.
245 Ten samples were prepared for Nd, Pb and Sr isotope ratios analyses. Two
246 sets of Sr samples, unleached and leached, were prepared following the same
247 procedures as for the Nd samples and Pb samples, respectively. The samples were
248 dissolved and conditioned in Savillex beakers. Rock chips were leached according to
249 McDonough and Chauvel (1991), to eliminate as much as possible Sr and Pb
250 superficial contamination. For Nd and unleached Sr isotopic measurements, 100 mg
251 of sample were dissolved using HNO3 and HF and isolated using the same
252 procedure as Chauvel et al. (2011). For Pb and leached Sr, 1 g of rock chips was
253 leached prior to dissolution using HCl and then isolated as in Chauvel et al. (2011).
254 Nd and Pb isotopic ratios were measured using a Nu Plasma HR MC–ICPMS at
10
255 ENS Lyon, France, while Sr isotopic ratios were measured using a Thermo Scientist
256 Triton MS at the University of Brest, France.
257
258 Results
259 Fission-track results
260 Anzá – Bolombolo section
261 The tuff layer at the bottom of the Anzá-Bolombolo section (sample JJ22) has
262 an AFT central age of 8.4±3.1 Ma, and the pyroclastic flow sampled towards the top
263 of the section (sample JJ13) has an AFT central age of 7.9±1 Ma (Table 1; see the
264 supplementary data for individual grain ages and radial plots of all samples). The
265 combined Combia Formation AFT data are shown in a radial plot in Figure 6A with a
266 central age of 8.6±1.4 Ma based on 302 grain ages.
267
268 La Metida Creek section
269 In total six samples were analyzed with the AFT method and ten with the ZFT
270 method. AFT central ages range between 15.9±11.1 and 5.1±2.5 Ma. Nonetheless,
271 inherited single grains with apparent cooling ages of between 374 and 49 Ma can
272 also be observed in all samples (Table 1). Zircon crystals were mainly found in the
273 middle and bottom of the La Metida Creek section. The euhedral to subhedral zircon
274 crystals range in color from colorless, yellow, pink to red. The ZFT central ages are
275 between 12.7±2.4 Ma and 6.1±1.1 Ma (Table 2). Except for the volcaniclastic
276 sandstone sample (JJ6), no strong evidence exist of contamination with inherited
277 zircons derived from surrounding country rock (see the supplementary data for
278 individual grain ages and radial plots of all samples). The combined Combia
11
279 Formation ZFT data are shown in Figure 6B with a central age of 9.1±1.1 Ma based
280 on 346 grain ages.
281
282 Petrographic results
283 Cerro Amarillo section
284 In general, the seven samples analyzed for this section share similar
285 characteristics being hypocrystalline, porphyritic rocks. The mineral assemblage is
286 represented by plagioclase + pyroxene ± amphibole ± olivine (Table 3). Other
287 minerals present in the samples are secondary calcite, biotite and opaque minerals.
288 The rock fragments found in the ignimbrites are mainly basalts (aphanitic textures
289 and volcanic glass) or andesites (plagioclase crystals in volcanic glass). Some of
290 these fragments are fractured. There is also evidence of oxidation and sericitization,
291 even though carbonate minerals are the main alteration product in these samples.
292 The ignimbrites are dominated by crystals and rock fragments ranging from
293 55 – 70 %, whereas the two basalt samples have different percentage relationships
294 between the matrix and phenocrysts, CA – 14 rich in crystals and CA – 18 rich in
295 matrix. The crystal and/or rock fragments are in-equigranular, which is observed in
296 the presence of seriate, glomeroporphyritic, poikilitic, and interstitial textures.
297 Overgrowth textures such as skeletal, corona and crystal zoning are also found in
298 the samples, mainly in the ignimbrites. The crystals have subhedral to anhedral
299 shapes in most samples; euhedral-shaped crystals are rare or unable to identify due
300 to alteration. The matrix is generally altered to secondary calcite, but in some cases
301 a non-altered volcanic glass composition is observed with some embedded
302 microlites of plagioclase and less common pyroxene.
12
303 Based on the lack of quartz and potassic feldspar, all samples from the Cerro
304 Amarillo section plot in the basalt/andesite field of the classification diagram of
305 Streckeisen (1976) shown in Figure 7A. Color plates of thin section photographs are
306 given in the supplementary data archive.
307
308 Anzá – Bolombolo section
309 The analyzed samples are hypocrystalline, un-equigranular volcanic rocks.
310 The mineral assemblages are mainly plagioclase + pyroxene (Table 3). The matrix
311 consists of volcanic glass. Other rock components are spherulites, found in samples
312 AB–6 and AB–7, and olivine, found in sample AB–6. These samples are located to
313 the east of the unconformity described in the stratigraphic section. The samples are
314 characterized by having skeletal and crystal zoning overgrowth, spherulites and
315 vesicular textures. The lava flows can be classified as basalt/andesite in the
316 Streckeisen (1976) diagram (Fig. 7a), and the pyroclastic flow deposits as crystal
317 tuffs after Pettijohn (1975), as shown in Figure 7b. Color plates of thin section
318 photographs are given in the supplementary data.
319
320 La Metida Creek section
321 Nine samples from this section mainly plot in the crystal tuff field of the
322 Pettijohn (1975) classification (Fig. 7b). Only one sample (QML – 9) is defined as
323 tuffaceous sandstone because of the presence of cross-bedding in the layer.
324 Petrographic characteristics of all samples are similar and the classification as
325 pyroclastic and epiclastic rocks is based on sedimentary structures observed in the
326 field. The mineral assemblage is mainly plagioclase + pyroxene. Some amphiboles
327 are present at the bottom layers.
13
328 The sampled rocks are mainly hypocrystalline due to the presence of
329 phenocryst, and microlites in the matrix. The minerals have un-equigranular and
330 seriate fabrics. In general, skeletal textures are found in all analyzed samples. Other
331 common textures are glomero-porphyritic and crystal zoning, although the latter is
332 not present in the samples analyzed from the middle section of the La Metida Creek
333 section. Similar to the Anzá-Bolombolo section spherulites are found in the samples
334 from the bottom layers. Color plates of thin section photographs are given in the
335 supplementary data.
336
337 Geochemical results
338 Mayor element analyses of 16 samples are presented in Table 4. Loss on
339 ignition (LOI) is generally below 3%. For the Cerro Amarillo section samples, SiO2
340 contents range between 51 and 53 wt%; they plot in the tholeiitic field of the AFM
341 diagram (Fig. 8A) and correspond to basaltic andesite according to Figures 8B.
342 Samples coming from the Anza-Bolombolo area have slightly higher SiO2 content at
343 about 56 wt%; they plot in the alkaline field in Fig. 8A and correspond to trachy-
344 andesites in Fig. 8B.
345 Trace element contents of all samples are given in Table 5 and plotted in
346 primitive mantle-normalized spider diagrams in Fig. 9A. The Cerro Amarillo samples
347 display an enrichment in large-ion lithophile elements (Rb, Ba, Cs, Sr) and a strong
348 depletion in Nb and Ta. The Anzá-Bolombolo samples are even more enriched in
349 Rb, Ba, Cs and Sr, and with similar depletion in Nb and Ta (Fig. 9A). The main
350 difference between the Cerro Amarillo and Anzá-Bolombolo samples is the Li
351 enrichment of the Anzá-Bolombolo section samples. Samples from both sections are
352 enriched in Light Rare Earth Elements (LREE) relative to the Heavy Rare Earth
14
353 Elements (HREE) (Fig. 9B) with a stronger fractionation in the Anzá-Bolombolo
354 section samples. No significant Eu anomaly exists for all samples.
355
356 Nd, Sr, and Pb isotope compositions
357 Nd, Sr, and Pb isotope analyses of all samples are given in Table 6. Strontium
358 isotopic ratios measured on leached and unleached samples are similar within
359 errors. 87Sr/86Sr ratios range from 0.703862 to 0.703931 for the Cerro Amarillo
360 section samples, but are higher at about 0.70417 for the Anzá-Bolombolo section
361 samples (Figure 10A). 143Nd/144Nd ratios vary between 0.51292 and 0.51298 for the
362 Cerro Amarillo section samples, and are somewhat lower at 0.51290 for the AB
363 section samples (Figure 10B and C). Finally, the Cerro Amarillo section samples
364 define a small range in Pb isotopic ratios (208Pb/204Pb: 38.68 to 38.80, 207Pb/204Pb:
365 15.61 to 15.62 and 206Pb/204Pb: 18.91 to 19.07), and the Anzá Bolombolo section
366 samples fall in the middle of the range (Figure 11a and b)
367
368
369 Discussion
370
371 Constraints from low-temperature thermochronology
372 The AFT and ZFT data presented in this study can in principle be used for
373 constraining the age of deposition of the volcanic and volcaniclastic deposits of the
374 Combia Formation (Kowallis et al., 1986; Bernet et al., 2016). The AFT and ZFT data
375 central age values ranging from 15.9 – 5.1 Ma for AFT and 12.7 – 6.1 Ma for ZFT,
376 bracket the known 12-6 Ma age of Combia Formation volcanic activity (e.g. Leal-
377 Mejía, 2011). Our fission-track data highlight two important aspects that are
15
378 challenging in dating relatively young volcanic and volcaniclastic deposits with the
379 fission-track method. As to be expected the ZFT data correspond more closely to the
380 known 12-6 Ma age range determined from zircon U-Pb analyses (Leal-Mejía, 2011),
381 because of the higher U concentration and the better track counting statistics
382 resulting in higher precision results. The AFT data suffer under the very low (in
383 general <10 ppm) U concentration of the apatites in the Combia Formation. As can
384 been seen in the single grain data provided in the supplementary data archive, many
385 apatite grains are zero-track grains, resulting in a very high single grain age
386 uncertainty, as the induced track counts also tend to be because of the low U
387 concentrations.
388 In addition, dealing with volcanic and particularly volcaniclastic deposits the
389 risk of contamination with apatites and zircons recycled from the country rock is high,
390 and has been shown to be the case for certain volcanic deposits of the Paipa-Iza
391 volcanic complex (Bernet et al., 2016). Here we also think that zircons with >12 Ma
392 apparent cooling ages were most likely recycled from the Amagá Formation
393 (Piedrahita et al., 2017). Pre-Miocene cooling ages are common in apatites of the
394 Combia Formation deposits (Table 1), and are considered to be derived from
395 underlying basement rock and recycling of the Amagá Formation.
396 In summary, based on the AFT and ZFT data, volcanic activity occurred
397 between 12 Ma and 6 Ma. The main phase of activity for these deposits may have
398 been at around 9 Ma, as suggested by the central ages of the combined AFT and
399 ZFT data sets shown in Figure 6. This confirms a late Miocene depositional age,
400 which has previously been proposed based on stratigraphic position and whole rock
401 K-Ar dating of hypabyssal porphyries (e.g. Grosse, 1926; Restrepo et al., 1981;
16
402 Marriner and Millward, 1984; González, 2001, Pérez, 2005; Ramírez et al., 2006;
403 Leal-Mejía, 2011).
404
405 Shallow-level processes prior to eruption
406 The results presented in this study indicate that there are two different
407 petrographic trends among the Combia Formation rocks. In general, the rocks have
408 porphyritic textures, and plagioclase is one of the main mineral components, both as
409 phenocrysts and microlites. Similar results have been reported by Marriner and
410 Millward (1984), López et al. (2006) and Ramírez et al. (2006).
411 The matrix for most samples is comprised of volcanic glass with microlites of
412 plagioclase and to a lesser extent pyroxene. Devitrification of the volcanic glass
413 matrix is common in the samples. The samples show evidence of alteration (e.g.
414 secondary calcite, oxidation, argillitization) which may indicate metasomatic to
415 surficial processes related to hydrothermal alterations and mineralization processes
416 in the hypabyssal porphyries of the study area (e.g. Tassinari et al., 2008; Leal-
417 Mejía, 2011; Lesage et al., 2013; Uribe-Mogollón, 2013).
418 All samples show disequilibrium textures such as skeletal, sieve and
419 spherulitic textures, embayments, reaction rims, coronas and crystal zoning. These
420 textures are attributed to different conditions and magmatic processes such as
421 pressure variations, zoned magma chambers, decompression, magma mixing,
422 phenocrysts recycling and fractional crystallization (e.g. Nixon and Pearce, 1987;
423 Nelson and Montana, 1992; Singer et al., 1995; Perugini et al., 2003; Aldanmaz,
424 2006; Maro and Remesal, 2011). Thus, our petrographic results favor mainly magma
425 mixing and fractional crystallization to be the main causes for disequilibrium in the
426 magma chamber.
17
427
428 Magma genesis
429 Magmatic arcs are the result of subduction of oceanic crust beneath
430 continental crust and this complex setting has impact on magmatic processes such
431 as partial melting, fractional crystallization, changes in pressure and temperature,
432 sediment melting, dehydration, and decarbonation (e.g. Rollinson, 1993; Albarade,
433 1995; White, 2013). In addition, fluids added to magma play an important role, as
434 fluids allow the transport of incompatible elements from the subducted oceanic
435 basalt and sediments to the magma, leading to enrichment in specific mobile
436 elements and modifying the isotopic composition of the asthenospheric magma
437 source (Tatsumi, 2005; Tatsumi and Stern, 2006; Tatsumi and Takahashi, 2006;
438 Nakamura et al., 1985).
439 Our new geochemical data for the Cerro Amarillo area are generally similar to
440 what was previously published by Marriner and Millward (1984) and by Ordoñez
441 (2001). Major elements allow identification of a tholeiitic trend in the samples from
442 the eastern Amagá basin while the samples from the western Amagá basin follow a
443 calc-alkaline trend (Fig. 8A). Both magma suites have been previously recognized at
444 other sampling sites of the Combia Formation (Fig. 8A; e.g. Álvarez, 1983; Marriner
445 and Millward, 1984; Ordoñez, 2001; Leal-Mejía, 2011). With SiO2 contents between
446 47 – 59 wt% our Cerro Amarillo samples plot in the basaltic andesite field of Fig. 8B
447 and the samples from Anzá Bolombolo plot in the trachy-andesite field of LeMaitre et
448 al. (1989) and Cox et al. (1979) (Fig. 8B). For comparison, published data for the
449 Combia Formation are also shown in this figure. It appears clearly that the AB
450 section samples from the western Amagá basin are much more alkaline than others
451 (Fig. 8B), and that samples from both sections have lower SiO2 contents than the
18
452 volcanic rocks of the 24-20 Ma magmatic phase and most of the 17-9 Ma magmatic
453 phase rocks analyzed by Leal-Mejía (2011). Despite these differences, so far no
454 precise division of the basin with respect to the magmatic suites can be given at the
455 moment, and more detailed mapping and geochemical analyses are necessary.
456 The trace elements provide clear evidence of a subduction-related
457 geochemical signature, with Nb and Ta depletion (e.g. Wilson, 1989; White, 2013).
458 Samples also all have very high Ba, U, Pb and Sr contents as already noticed for
459 older samples from the Combia Formation (Fig. 9C, Leal-Mejía, 2011 data
460 summarized in Marín-Cerón et al., 2019). Medium to slightly elevated Ba/Th values
461 (a proxy for slab dehydration Fig. 9E; Labanieh et al., 2012) characterize the Cerro
462 Amarillo samples from the eastern Amagá basin, whereas the AB samples of the
463 western Amagá basin have low ratio consistent with a sediment melting trend.
464 In general, the trace element results of the Amagá basin resemble those of
465 the northern volcanic zone (NVZ) of the Andes, as summarized in Marín-Cerón et al.
466 (2019), even though the Combia Formation has higher LILE (Rb, Sr, Ba) contents
467 and lower Nb and Ta contents than those reported for the NVZ (Thorpe et al., 1982;
468 Marriner and Millward, 1984).
469 The REE patterns of samples from the Anza Bolombolo and Cerro Amarillo
470 sections are somewhat different, with higher fractionation in the former group (Fig.
471 9b). In comparison to the REE spectra of the 17-6 Ma porphyritic intrusions and
472 recent volcanism, the Combia Formation shows a pattern closer to the latest stage of
473 volcanic activity (Fig. 9D; data from Leal-Mejía (2011), summarized by Marín-Cerón
474 et al. (2019)). The difference in the slope of the REE patterns of eastern and western
475 Amagá basin samples suggest differences in terms of magma formation, most
476 probably during melting processes in the mantle source. Overall, the absence of Eu
19
477 anomaly suggests that melting occurred relatively deep, below the plagioclase
478 stability level (~40 km depth).
479
480 Magma source composition
481 Combining trace element data with isotopic data can help understanding the
482 origin of magmas and the potential role of subducted slab addition to the mantle
483 wedge (e.g Tatsumi, 2005; Tatsumi and Stern, 2006). The Cerro Amarillo and Anzá-
484 Bolombolo samples have medium to slightly elevated Sr/Th and rather low 87Sr/86Sr
485 ratios (Fig. 10A), indicating transfer of elements from the subducted slab byNVZ
486 aqueous fluids. Because no systematic difference in 87Sr/86Sr is observed between
487 leached and unleached samples (Table 6), post-emplacement alteration can be
488 excluded, and the measured ratios can be considered as representative of the
489 magma source (e.g. Tamura and Nakamura, 1996; Shibata and Nakamura, 1997).
490 Similarly, the large range of Ba/Th at almost constant 143Nd/144Nd indicates addition
491 of Ba through slab dehydration (Fig. 10B), with a stronger effect in the eastern
492 Amagá basin than in the western part of the basin. In a 87Sr/86Sr vs 143Nd/144Nd
493 isotopic space (Fig. 10C), the Amaga basin samples fall as expected within the field
494 defined by the NVZ (see compilation of Marín-Cerón et al., 2019). It is worth noting
495 that the Amaga Basin samples correspond to the most depleted part of the isotopic
496 range observed along the Andes, suggesting limited crustal contamination during
497 magma ascent and/or limited contribution of subducted sedimentary material to the
498 mantle wedge. It is also worth noting that the Anzá-Bolombolo samples have slightly
499 more enriched isotopic characteristics than the Cerro Amarillo samples, a feature
500 consistent with the difference seen in Figure 9E since sediment addition tends to
501 lower the Nd isotopic composition and increase the Sr isotopes.
20
502 Lead isotopes provide complementary and useful information. As was the
503 case for Sr and Nd isotopic data, the Amaga basin samples fall in the field defined by
504 the northern volcanic zone and differ drastically from fields defined by central and
505 southern volcanic zones (Fig. 11A) (see compilations made by Marín-Cerón, 2007
506 and Marín-Cerón et al., 2010; 2019). The rather radiogenic values of Pb isotopes for
507 the northern volcanic zone have been interpreted as being due either to an enriched
508 mantle reservoir or to continental crust assimilation. The enriched mantle hypothesis
509 was suggested by Rodríguez-Vargas et al. (2005) on the basis of the Nd and Sr
510 isotopic characteristics of xenoliths from the Mercaderes region in SW Colombia.
511 The authors invoked the potential involvement of magma material coming from the
512 Galapagos plume, but such influence under the Amaga basin seems quite unlikely
513 given the distance between the SW Colombian arc and the Galapagos (>450 km,
514 Pedersen and Furnes, 2001). However, the Amaga Basin samples analyzed in this
515 study provide new information because they define a tight correlation in 208Pb/204Pb
516 vs 206Pb/204Pb space (see Fig 11B). Such linear array implies the involvement and
517 mixture of two endmembers whose compositions remain unchanged during the
518 entire volcanic sequence. The enriched end-member seems to correspond to the
519 local lower continental crust (see Fig. 11B) while the less radiogenic endmember is
520 more ambiguous. Following Marin-Ceron’s model (2019), this ‘depleted’ endmember
521 could correspond to the mantle wedge whose composition would be affected by the
522 presence of material originating from the subducted slab (see Fig. 11B).
523 Nonetheless, there might be differences in the subduction mechanisms, proportion of
524 end-members interaction, and magma source evolution between magmatism at 12 –
525 6 Ma and magmatism at 3 Ma – present, despite assuming the same end-members.
526 In summary, magma was generated by slab dehydration, sediment melting and
21
527 interactions with the LCC, resulting in the mixing of at least two end-member
528 sources. Due to differences in depth of melting and other magmatic processes (AFM
529 and MASH), as shown in Figure 12, the late Miocene volcanic rocks of the western
530 and eastern Amagá basin show distinct petrologic and geochemical signatures.
531
532 Conclusions
533 The late Miocene volcanic and volcanoclastic Combia Formation of the
534 Amagá basin between in the Central and Western Cordillera developed above the
535 Nazca plate subduction zone in western Colombia. Volcanic and volcaniclastic rocks
536 of the Combia Formation are characterized by a sequence of ignimbrites and lava
537 flows of tholeiitic affinity at the bottom and pyroclastic flows to the top of the
538 formation in the eastern Amaga basin and a succession of pyroclastic and epiclastic
539 flows with calc-alkaline affinity in the western Amagá basin. Using apatite and zircon
540 fission-track dating the timing of volcanic activity during the deposition of the Combia
541 Formation was confirmed between 12 and 6 Ma.
542 Trace element, REE and Nd, Sr and Pb isotopic analyses show that the
543 surface weathering did not modify the geochemical signatures and that the
544 geochemical composition of the samples results of several magmatic processes
545 including slab dehydration and sediment melting to form the primary magma in the
546 mantle wedge and mixing of this primary magma with lower continental crustal
547 before eruption. In contrast, contamination by upper crustal rocks could not be
548 detected. Finally, the new geochemical results confirm that volcanism in the Combia
549 area between 12 and 6 Ma was similar to what is known about the NVZ of the Andes
550 in South America.
551
22
552
553 Acknowledgements
554 We acknowledge support of this study from ECOS-NORD/Colciencias/ICETEX 555 project C12U01 of M. Bernet and M.I. Marín-Cerón, as well as a BQR SUD grant at 556 ISTerre, awarded to M. Bernet. We thank Wilton, Francois Senebier and Francis 557 Coeur for help with sample preparation and mineral separation.
558
559
23
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889
890
891 Figure captions
892 Fig. 1 Overview map of the Colombia Andes, showing the subduction of the Nazca 893 and Caribbean plates beneath the South American plate. Also shown are the
38
894 Western, Central and Eastern Cordilleras and areas of Pliocene to present volcanic 895 activity, as well as the location of the study area (map from GeoMapApp, 896 http://www.geomapapp.org/).
897 Fig. 2 Geological map of the Amagá basin with the locations of the Cerro Amarillo 898 (CA), Anzá-Bolombolo (AB) and La Metida Creek (MC) sections (modified after 899 Sierra and Marín-Cerón, 2011).
900 Fig. 3 Cerro Amarillo stratigraphic of the eastern Amagá basin.
901 Fig. 4 Anzá Bolombolo stratigraphic section of the western Amagá basin.
902 Fig. 5 La Mertida Creek stratigraphic section of the western Amagá basin.
903 Fig. 6 Combined fission-track data radial plots of A) apatite fission-track data and B) 904 zircon fission track data with central ages.
905 Fig. 7 A) Streckeisen (1976) volcanic rock classification diagram. Both the Anzá- 906 Bolombolo and Cerro Amarillo samples plot in the andesite, basalt field. B) 907 Pyroclastic rock classification diagram of Pettijohn (1975), in which almost all La 908 Metida Creek and Anzó-Bolombolo pyroclastic rock samples plot in the crystal tuff 909 field.
910 Fig. 8 A) AFM diagram plot (Irvine and Baragar, 1971) for volcanic rocks from the 911 Cerro Amarillo and Anzá- Bolombolo sections. For comparison, data of Marriner and 912 Millward (1984), Ordoñez (2001) and Leal-Mejía (2011) from the Combia Formation 913 are also shown. B) Total alkalis versus silica (TAS) diagram of volcanic rocks from 914 the Cerro Amarillo and Anzá Bolombolo sections; boundaries in the total alkalis are 915 from LeMaitre et al. (1989) for rock classification and Irvine and Baragar (1971) for 916 magma series classification (red solid line). For comparison, data of Marriner and 917 Millward (1984), Ordoñez (2001) and Leal-Mejía (2011) are shown.
918 Fig. 9 A) Primordial mantle (McDonough and Sun, 1995) normalized trace element 919 spider diagrams of volcanic rocks from the Cerro Amarillo and Anzá-Bolombolo 920 sections. B) Chondrite (Evensen et al., 1978) normalized Rare Earth Element (REE) 921 patterns of the volcanic rocks from the Cerro Amarillo section. C) For comparison 922 trace element patterns of published data by Leall-Mejia (2011) from Combia 923 Formation and hypabyssal porphyritic intrusions in the study area, as summarized in
39
924 Marín-Cerón et al. (2019). Trace element data normalized after Wood et al. (1979). 925 D) For comparison, published REE data of Leal-Mejía (2011) normalized after Sun 926 and McDonough (1989) for hypabyssal porphyritic intrusions, Combia Formation 927 volcanic rocks and recent to present volcanism in the Central Cordillera, as 928 summarized in Marín-Cerón et al. (2019). E) The La/Sm versus Ba/Th plot indicates 929 that the Cerro Amarillo volcanic rocks were more derived from magma related to slab 930 dehydration, whereas the Anzá-Bolombolo samples trend more towards sediment 931 melting derived magma.
932 Fig. 10 Comparison between trace elements and isotopic systematics: A) Sr/Th 933 versus 87Sr/86Sr, and B) Ba/Th versus 143Nd/144Nd, for volcanic rocks of the CA 934 section (blue circles) and the AB section (red circles). The dashed line represents 935 altered oceanic crust values (AOC) (after Barret, 1983). Both diagrams show that 936 addition of fluids to the magma affected the geochemistry to the analyzed rocks and 937 that the slab dehydration effects are more pronounced in the eastern than the 938 western Amagá basin. C) Nd vs. Sr isotope ratio plot, showing the fields for the 939 Northern Volcanic Zone (NVZ), Central Volcanic Zone (CVZ) and Southern Volcanic 940 Zone (SVZ) as well as typical MORB composition, based on data from James et al. 941 (1976); Hawkesworth et al. (1979); James (1982); Harmon et al. (1984); Frey et al. 942 (1984); Thorpe (1984); Hickey et al. (1986); Hildreth and Moorbath (1988); Wörner et 943 al. (1988); Walker et al. (1991); de Silva (1991); Kay et al. (1991); Davidson and de 944 Silva (1992). Winter (2001); Marín-Cerón (2007), as summarized by and plot 945 modified from Marín-Cerón et al. (2019). The data of our study are shown for the 946 Cerro Amarillo section (yellow circles) and the Anzá-Bolombolo section (red circles), 947 plotted over the NVZ field.
948 Fig. 11 Lead isotopic systematics of the Combia Formation shown for the Cerro 949 Amarillo section (yellow circles) and the Anzá-Bolombolo section (red circles). A) 950 Plots of 208Pb/204Pb vs 206Pb/204Pb for the Andean volcanic zones (Northern Volcanic 951 Zone – NVZ; Central Volcanic Zone – CVZ; and Southern Volcanic Zone – SVZ) and 952 the pre-Andean basement (plot modified from data compilation plot of Marín-Cerón 953 (2019). Pacific sediments (Dasch, 1981; White et al., 1985); Paleozoic basement 954 (Chiaradia and Fontboté, 2002); metalliferous sediments from DSDP leg 92 (Barret 955 et al., 1987). B) Zoom on the 208Pb/204Pb vs 206Pb/204Pb diagram. Squares represent 956 possible end-members and the respective trends of the interaction between each of
40
957 the components involved during magma formation. AOC: altered oceanic crust; HS: 958 hemipelagic sediments; CS: carbonaceous sediments; LCC: lower continental crust. 959 The solid blue line represents the linear trend of the samples suggesting bimodal 960 mixing between primary magma (yellow star) and LCC. This plot is based on the 961 compilation of Marín-Cerón et al. (2019); Cretaceous Domain (Kerr, 2003); Lower 962 crust xenotiths (Weber et al., 2002); and ACC from Hole 504 (Pedersen and Furnes, 963 2001); NVZ data from Marín-Cerón (2007). The data from our study study are shown 964 for the Cerro Amarillo section (yellow circles) and the Anzá-Bolombolo section (red 965 circles) and the plotted over the Northern Volcanic Zone field.
966 Fig. 12 Schematic diagram for magma source genesis of Combia Formation 967 volcanism. AOC: altered oceanic crust; HS: hemipelagic sediments; CS: 968 carbonaceous sediments; AFC: assimilation fraction crystallization processes 969 (DePaolo, 1981); MASH: melting, assimilation, storage, and homogenization 970 processes (Hildreth & Moorbath, 1988); LCC: lower continental crust; UCC: upper 971 continental crust. Illustration based on model proposed for southwestern Colombian 972 volcanism (Marín-Cerón, 2007) and is compatible with models presented in Marín- 973 Cerón et al. (2019).
974
975
976 Tables
977 Table 1 Apatite fission-track data of the Combia Formation
978 Table 2 Zircon fission-track data of the La Metida Creek Formation
979 Table 3 Petrographic modal analyses
980 Table 4 Major elements (wt%) of the Cerro Amarillo and Anzá-Bolombolo section 981 samples
982 Table 5 Trace elements (ppm) of volcanic rock samples of the Cerro Amarillo and 983 Anzá-Bolombolo sections
984 Table 6 Isotopic compositions of volcanic rocks from the Cerro Amarillo and Anzá- 985 Bolombolo sections.
41
986 Table 7 Estimated isotopic compositions and parameters for end-member involved in 987 magma genesis
42
Table 1 Apatite fission‐track data of the Combia Formation
Number Single grain Age Central Sample RhoS RhoI RhoD U (ppm) Lithology of age range Ns Ni P(χ2) (%) dispersion age* (Ma) number (x105t/cm2) (x105t/cm2) (x105t/cm2) ±2 SE grains (Ma) (%) ±2 SE AB section
Pyroclastic JJ13 60 2.8 – 36.9 0.28 67 4.88 1183 9.72 44.9 2.7 7.9±2.1 6±0 agglomerate
JJ22 Tuff 35 3.2 – 38.5 0.29 35 4.96 592 9.72 36.3 24.0 8.4±3.1 7±1
MC section
JJ17 Lapilli – tuff 60 3.6 – 71.5 0.26 36 4.57 624 9.72 7.3 50.8 8.3±3.1 6±0
JJ14 Tuff 33 4.9 – 374.9 0.29 18 3.34 209 9.72 0.0 141.1 15.9±11.1 4±1
JJ21 Tuff 51 3.5 – 74.2 0.17 19 4.56 517 9.72 66.9 2.0 5.1±2.5 6±1
Volcaniclastic JJ18 16 4.7 – 48.9 0.23 7 4.59 139 9.72 0.9 155.4 7.3± 9.4 6±1 sandstone
JJ19 Tuff 20 6.6 – 138.7 0.24 10 3.23 133 9.72 45.7 2.1 10.5±7.3 4±1
JJ20 Lapilli tuff breccia 27 4.9 – 138.5 0.50 28 5.68 317 9.72 6.9 57.1 15.8±9.2 9±1
combined 302 2.8‐374.9 9.72 0.0 48.6 8.6±1.4 6±0
Note – RhoS: spontaneous track density. RhoI: induced track density; P(χ2): Chi2 probability. Fission‐track ages were calculated using a Zeta value of 288.36±7.90. AFT data calculated with Binomfit of Brandon (see Ehlers et al., 2005).
Table 2 Zircon fission‐track data of the La Metida Creek Formation
Number Single grain Age Central Sample RhoS RhoI RhoD P(χ2) U (ppm) Lithology of age range Ns Ni dispersion age* (Ma) number (x105t/cm2) (x105t/cm2) (x105t/cm2) (%) ±2 SE grains (Ma) (%) ±2 SE Lapilli tuff JJ1 30 1.0 – 14.3 4.65 175 17.6 662 2.71 24.4 24.2 6.7±1.5 258±21 breccia
JJ8 Tuff 12 2.1 – 19.4 5.89 58 24.1 237 2.67 3.3 44.3 6.2±2.6 359±47
JJ3 Tuff 25 4.0 – 19.5 10.6 383 27.5 993 2.71 47.5 6.6 10.0±1.7 405±28
JJ9 Tuff 28 0.9 – 25.5 13.2 570 33.1 1432 2.67 0.0 35.3 10.1±2.1 493±29
JJ10 Tuff 22 5.0 – 20.0 10.5 363 28.6 989 2.66 68.0 0.6 9.3±1.5 427±29
JJ4 Tuff 31 2.9 – 25.8 17.7 585 38.8 1280 2.70 0.3 24.1 11.2±2.0 572±36
Volcaniclastic JJ6 51 2.9 – 46.7 10.6 909 22.1 1844 2.69 0.0 44.1 12.7±2.4 327±17 sandstone
JJ5 Tuff 31 2.6 – 14.8 14.1 515 3.85 1405 2.69 73.1 6.5 9.4±1.4 569±14
Lapilli tuff JJ11 48 1.3 – 16.1 6.27 362 2.63 1517 2.65 14.2 19.6 6.1±1.1 394±22 breccia
Lapilli tuff JJ7 68 4.3 – 14.8 9.00 824 29.5 2705 2.68 94.0 0.7 7.8±1.1 439±20 breccia
Combined 346 0.9 – 46.7 10.2 4744 28.5 13206 2.68 0.0 33.9 9.1±1.1 418±14
Note – RhoS: spontaneous track density. RhoI: induced track density; P(χ2): Chi2 probability. Fission‐track ages were calculated using a Zeta value of 191.6±10.25. ZFT data calculated with Binomfit of Brandon (see Ehlers et al., 2005).
Table 3 Petrographic modal analyses CA section CA - 1 CA – 2 CA – 7 CA – 13 CA - 14 CA - 18 CA - 22 Plagioclase 48.61 19.1 36.2 9.25 32.1 89.7 31.2 Hypersthene --- 42.2 23.5 51.2 47.2 10.3 21.8 Augite 13.19 4.7 3.2 9 9.89 --- 9.5 Hornblende 3.47 0.6 ------5.4 Calcite 9.03 1.3 ------7.58 --- 5.01 Olivine 5.21 ------8 Biotite --- 0.5 0.32 1 3.23 --- 1.6 Sericite ------3.5 ------Rock fragments 19.8 19.4 28.6 29.55 ------17.49 Oxides --- 8.8 4.8 ------Opaque minerals 0.69 3.4 ------Total 100 100 100.12 100 100 100 100 AB section AB – 2 AB – 6 AB – 7 Plagioclase 57.14 69.13 52.22 Pyroxene 42.86 12.01 29.1 Spherulites --- 9.86 18.68 Olivine --- 9 --- Total 100 100 100 MC section QML - 1 QML – 6 QML - 7 QML – 9 QML – 10 QML - 14 QML - 18 QML - 22 QML - 28 QML - 31 Plagioclase 71.22 61.4 55 40 57.14 85 57.5 62.5 60 77.14 Pyroxene --- 10.53 15 20 22.85 7.6 25 25 25 14.29 Hornblende 5.91 5.26 5 ------2.4 ------Biotite 0.33 ------Oxides 2.13 ------5.71 5.72 5 --- 12.5 15 8.57 Rock fragments 16.48 15.79 --- 8.57 ------Opaque minerals 3.94 7.02 25 25.72 14.29 ------Spherulites ------17.5 ------Total 100.01 100 100 100 100 100 100 100 100 100
Table 4 Major elements (wt %) of the Cerro Amarillo and Anzó – Bolombolo section samples
Oxides JJ2‐1‐ JJ2‐1‐ JJ1 ‐ 3 JJ1 ‐ 6 JJ1 – 9 JJ1 ‐ 13 JJ1 ‐ 17 JJ1 – 18 JJ1 ‐ 20 JJ1 ‐ 23 JJ3 – 2 JJ3 ‐ 5 JJ3 ‐ 6 JJ3 ‐ 9 JJ4 ‐ 2 JJ4 ‐ 3 (wt %) 10 14
SiO2 53.20 52.68 52.56 52.62 52.55 52.10 52.49 52.64 52.09 51.19 52.07 52.22 51.78 52.34 55.45 55.78
Al2O3 14.80 14.70 14.82 14.71 14.66 14.61 14.59 14.87 18.30 15.29 15.05 15.22 17.49 17.66 19.02 18.93
Fe2O3 t 12.03 11.77 12.13 12.82 12.67 12.55 12.93 12.75 10.40 13.44 13.48 13.63 10.49 10.23 5.01 5.53 MnO 0.19 0.17 0.17 0.19 0.19 0.18 0.19 0.18 0.18 0.21 0.21 0.21 0.17 0.17 0.09 0.09 MgO 3.56 3.51 3.32 3.48 3.43 3.32 3.49 3.30 2.99 3.44 3.50 3.46 3.48 3.05 1.05 1.12 CaO 7.68 7.82 7.56 7.57 7.58 7.47 7.36 7.50 9.33 8.28 8.35 8.24 8.80 8.84 4.51 5.28
Na2O 2.95 2.74 2.63 2.60 2.69 2.70 2.76 2.80 2.66 2.76 2.89 2.80 2.94 2.98 3.58 3.73
K2O 1.89 1.75 1.94 1.88 1.98 1.84 1.79 1.82 1.20 1.40 1.25 1.45 1.47 1.48 3.58 4.60
TiO2 1.31 1.30 1.38 1.39 1.38 1.38 1.38 1.38 0.86 1.03 1.06 1.06 0.96 0.99 5.10 0.52 P2O5 0.48 0.48 0.50 0.50 0.51 0.52 0.51 0.28 0.39 0.39 0.39 0.44 0.46 0.47 0.49 LOI 1.48 2.75 2.60 2.19 1.77 1.98 1.47 1.74 1.12 1.63 1.63 1.65 2.08 2.31 5.18 2.70 SUM 99.67 99.11 99.95 99.4 98.64 98.97 99.49 99.41 99.06 99.88 100.33 100.1 100.51 98.45 98.77 99.67
Table 5 Trace elements (ppm) of volcanic rock samples of the Cerro Amarillo and Anzó Bolombolo sections.
JJ1‐3 JJ1‐6 JJ1‐9 JJ1‐13 JJ1‐17 JJ1‐18 JJ1‐20 JJ1‐23 JJ3‐2 JJ3‐5 JJ3‐6 JJ3‐9 JJ4‐2 JJ4‐3 JJ2‐1‐10 J22‐1‐14
Li 8.52 8.33 7.58 8.46 8.73 9.75 8.71 10.4 8.98 8.76 7.64 9.39 8.07 8.38 13.6 15.5
Sc 31 30.7 30.2 30.5 30.1 29.5 30.1 30.4 27.4 33 32.8 33.1 24 24.8 8 8.75
Ti 7840 7760 8270 8340 8210 8110 8250 8240 5070 6170 6160 6200 5690 5900 2710 3020
V 343 340 367 369 361 365 366 367 296 331 338 337 268 278 96.9 100
Cr 12.7 11.6 13.5 13.1 13.2 13.5 13.5 13.3 10.9 15.7 16.5 17.2 31.4 32.6 1.4 1.02
Co 33.1 30.7 33.7 34.5 34.9 35.2 34.7 35.5 25.4 34.7 34.2 35.6 28 26.3 9.58 11.8
Ni 14.9 13 16 16.5 17.1 17.3 16.6 18 7.18 9.99 9.79 10.3 20.2 17.7 2.35 2.63
Cu 224 203 227 220 223 240 226 238 127 184 169 179 191 187 117 143
Zn 107 136 116 120 114 116 115 116 86.6 111 112 114 100 96.9 70.3 74.2
As 25.1 6.22 6.78 3.1 7.12 10.5 6.82 8.08 3.19 4.37 4.68 4.61 5.37 5.99 4.38 3.9
Rb 43.9 42.3 49.9 51.4 49.2 51.5 49.3 50.1 25.8 32.9 34.7 34 37.2 38.3 169 130
Sr 475 478 470 457 459 461 453 457 558 497 457 473 483 489 1870 1170
Y 26 26 28 27.5 27.2 27.6 27.3 27.4 18.9 23.3 23.5 24 21 22.2 15.5 17
Zr 110 108 116 115 114 116 114 115 55.7 75 76.2 77 65.7 68.5 106 118
Nb 5.97 5.83 6.18 6.25 6.11 6.26 6.19 6.16 2.63 3.03 3.07 3.06 3.05 3.16 4.86 5.54 JJ1‐3 JJ1‐6 JJ1‐9 JJ1‐13 JJ1‐17 JJ1‐18 JJ1‐20 JJ1‐23 JJ3‐2 JJ3‐5 JJ3‐6 JJ3‐9 JJ4‐2 JJ4‐3 JJ2‐1‐10 J22‐1‐14
Cd 0.0498 0.108 0.0574 0.0541 0.0487 0.0538 0.055 0.058 0.0441 0.0513 0.0469 0.0488 0.045 0.0461 0.0391 0.049
Cs 1.51 1.73 1.86 1.97 1.76 1.96 1.84 2 0.884 1.12 1.23 1.19 1.35 1.59 3 1.11
Ba 967 948 1030 990 1030 1010 1000 1010 607 842 823 847 717 742 1350 1250
La 10.5 10.5 11.2 11.2 11.1 11.3 11.2 11.2 5.7 7.46 7.54 7.62 7.14 7.39 19.7 21.4
Ce 22.7 22.6 23.9 24.3 23.8 24 23.9 23.9 12.4 16.2 16.4 16.5 15.4 15.7 36.5 39.9
Pr 3.21 3.21 3.42 3.46 3.36 3.42 3.41 3.41 1.83 2.39 2.41 2.42 2.22 2.29 4.69 5.13
Nd 14.7 14.6 15.5 15.8 15.5 15.7 15.4 15.4 8.64 11.3 11.5 11.7 10.3 10.7 18.4 20.2
Sm 3.87 3.94 4.24 4.29 4.16 4.2 4.25 4.18 2.48 3.24 3.33 3.37 2.81 2.92 3.74 4.13
Eu 1.21 1.23 1.27 1.27 1.26 1.28 1.28 1.24 0.858 1.09 1.07 1.1 0.98 1.04 1.2 1.29
Gd 4.53 4.46 4.74 4.71 4.73 4.67 4.66 4.73 2.96 3.87 3.92 3.96 3.34 3.52 3.3 3.59
Tb 0.713 0.717 0.747 0.758 0.745 0.754 0.755 0.753 0.479 0.623 0.645 0.66 0.542 0.58 0.456 0.487
Dy 4.5 4.55 4.65 4.77 4.68 4.85 4.78 4.78 3.19 4.08 4.18 4.23 3.58 3.77 2.54 2.84
Ho 0.925 0.929 1 1.01 0.984 0.986 0.975 0.984 0.665 0.844 0.869 0.868 0.746 0.789 0.503 0.548
Er 2.75 2.65 2.84 2.89 2.84 2.89 2.86 2.87 1.99 2.48 2.53 2.57 2.23 2.32 1.44 1.62
Tm
Yb 2.53 2.55 2.64 2.71 2.64 2.69 2.65 2.67 1.87 2.32 2.36 2.4 2.13 2.18 1.39 1.59 JJ1‐3 JJ1‐6 JJ1‐9 JJ1‐13 JJ1‐17 JJ1‐18 JJ1‐20 JJ1‐23 JJ3‐2 JJ3‐5 JJ3‐6 JJ3‐9 JJ4‐2 JJ4‐3 JJ2‐1‐10 J22‐1‐14
Lu 0.375 0.368 0.397 0.403 0.394 0.398 0.394 0.395 0.271 0.331 0.347 0.349 0.313 0.329 0.211 0.239
Hf 2.99 2.92 3.17 3.18 3.15 3.15 3.1 3.12 1.61 2.18 2.25 2.27 1.81 1.87 2.55 2.81
Ta 0.368 0.37 0.39 0.39 0.388 0.392 0.385 0.384 0.166 0.191 0.189 0.194 0.192 0.193 0.282 0.303
Tl 0.298 0.234 0.322 0.36 0.361 0.297 0.245 0.272 0.2 0.268 0.317 0.222 0.282 0.297 0.351 0.138
Pb 9.64 9.7 10.2 10.5 10.1 10.2 10.2 10.1 6 9.58 9.9 9.67 4.63 4.74 10.9 12.1
Th 1.98 1.97 2.07 2.11 2.06 2.1 2.08 2.09 1.03 1.39 1.4 1.41 1.19 1.23 4.46 4.95
U 1.08 1.08 1.18 1.11 1.12 1.11 1.1 1.11 0.517 0.854 0.857 0.843 0.528 0.532 1.22 2.19
Table 6 Isotopic compositions of volcanic rocks from the Cerro Amarillo and Anzó Bolombolo sections.
JJ1‐3 JJ1‐9 JJ1‐17 JJ1‐23 JJ3‐2 JJ3‐5 JJ3‐9 JJ4‐2 JJ2‐1‐10 JJ2‐1‐14
87Sr/86Sr 0.703911 0.703930 0.703931 0.703921 0.703916 0.703876 0.70387 0.703862 0.70417 0.70416
2σ 0.000006 0.000008 0.000008 0.000008 0.000006 0.000006 0.000006 0.000006 0.000006 0.000006
87Sr/86Sr 0.70391 0.70393 0.70393 0.70393 0.70392 0.70388 0.70387 0.70387 0.70417 0.70417 (leached)
2σ 0.000006 0.000006 0.000006 0.000008 0.000006 0.000006 0.000006 0.000006 0.000006 0.000006
143Nd/144Nd 0.51294 0.51293 0.51292 0.51295 0.51293 0.51296 0.51293 0.51298 0.51290 0.51289
2σ 0.000009 0.000018 0.000017 0.000010 0.000010 0.000007 0.000013 0.000008 0.000007 0.000010
εNd 5.959 5.930 5.684 6.223 5.846 6.420 5.905 6.882 5.255 5.191
208Pb/204Pb 38.72422 38.73927 38.73610 38.73702 38.71385 38.67951 38.68273 38.79674 38.74386 38.75921
2σ 0.00418 0.00418 0.00418 0.00418 0.00418 0.00417 0.00417 0.00418 0.004179 0.004180
207Pb/204Pb 15.61989 15.62459 15.62410 15.62365 15.62449 15.61989 15.62098 15.61286 15.60328 15.61037
2σ 0.00167 0.00167 0.00167 0.00167 0.00167 0.00167 0.00167 0.00167 0.001668 0.001669
206Pb/204Pb 18.96667 18.97333 18.97308 18.97264 18.93568 18.91002 18.91054 19.06522 19.00789 19.018005
2σ 0.00365 0.00365 0.00365 0.00365 0.00365 0.00364 0.00364 0.00367 0.003662 0.003666
Table 7 Estimated isotopic compositions and parameters for end‐member involved in magma genesis 208Pb/204Pb 206Pb/204Pb Pb (ppm) 142Nd/144Nd Nd (ppm) 87Sr/86Sr Sr (ppm)
AOC1,9 38.14 18.59 0.53 0.51280 4.71 0.70381 61.40
HS2,3,4 38.86 18.64 9.59 0.51247 17.0 0.70763 336.16
CS2,3,4,5 38.16 18.46 3.70 0.51242 0.89 0.70858 1 504.12
SC_1* 38.62 18.62 1.43 0.51285 5.94 0.70454 75.138
SC_2* 38.57 18.60 1.54 0.51284 1.15 0.70661 146.412
MW6,7 37.90 18.50 0.02 0.51310 0.71 0.70270 9.80
PM* 38.45 18.59 0.82 0.51307 5.81 0.70469 114.95
LCC8 38.73 19.02 8.81 0.51309 9.50 0.70423 173.00
* Estimated values. Kd from Halliday et al. (1995). AOC: Altered oceanic crust; HS: Hemipelagic sediments; CS: Carbonaceous sediments; SC_1: Subduction component 1 (AOC+HS); SC_2: Subduction component 2 (SC_1 + CS); MW: Mantle wedge (5%cpx, 25%opx, 70%ol); PM: Primary magma; and LCC: Lower continental crust. Values are calculated based on procedures followed by Marín‐Cerón (2007) for the SW Colombian volcanic arc. Values for AOC, HS, CS, MW, and LCC, are given according to data presented by Marín‐Cerón (2007). SC_2 represents the interaction between AOC (85%) and sediments (HS – 10% and CS – 5%). PM is calculated assuming 40% of metasomatized mantle by subduction component. It is considered 10% of LCC interacts with primary magma for magma source genesis. 1Pedersen et al. (2001); 2Plank and Langmuir (2000); 3Patiño et al. (2000); 4Vervoort et al. (1999); 5Hemming and McLennan (2001); 6Salters and Stracke (2004); 7Saunders et al. (1988); 8Weber et al. (2002); 9 10 Barret (1983); and Halliday et al. (1995).
12°N Caribbean plate
11°N
10°N
9°N Panama Venezuela
8°N Colombia
7°N Medellín AB South Nazca plate MVB Study American 6°N 6 cm/yr area Fig. 2 plate EC Paipa-Iza Nevado del Ruiz 5°N WC CPB Nevado Bogotá del Tolima EC = Eastern Cordillera CC = Central Cordillera Cerro Machin 4°N Nevado WC = Western Cordillera de Huila AB = Antioquia batholith CC CPB = Cauca-Patia basin 3°N MVB = Magdalena Valley Azufral Cumbal basin 81°W 80°W 79°W 78°W 77°W 76°W 75°W 74°W 73°W 72°W 71°W 70°W 69°W
Fig. 1 Bernet et al. Paleozoic Mesozoic Cenozoic Lithological units Jurassic CretaceousOligocene-Miocene Quaternary CA =CerroCA Amarillo MC =LaMetdiaCreek AB =Anzá andBolombolo Pgnp Kida Kdhb Kdha Kcdu Ksga Png Peni Pbsd Ksta Kgh Tmc Tdsa Tada Tadh PEa Pei Pes Pev TRa Jdp Jgr Jus Kaa Kuh Ksc Kvc Kvb Kg Tdc Toi Tos Tsc Qt Qtl Qd Qar Td Caldas amphibolite Migmatite La Iguanamicaceous gneiss Ayurá Gr. Montebello interbedded Ayurá Gr. Montebello phyllite Ayurá Gr. Montebello green schists Ayurá Gr. Montebello clastictexture Palmitas gneissic granite Amagá stock Pueblito diorite Roneral gabbro Ultramafic rocks Altavista batholith Penderisco Fm Ultramafic harzburgite Quebradagrande Fm. memeber sedimentary Quebradagrande Fm. volcanic memeber Barroso Fm. Heliconia hornblendediorite Heliconia quartzdiorite Antioquia batholith Altamira gabbro gabbroHispania Ursula stock Camburmbia stock Lower AmagáFm. Upper AmagáFm. Combia Fm. volcanic member Combia Fm. volcaniclastic member Andesitic dikesandsills porphyry Augite-andesitic Andesitic porphyry Dacitic porphyry Depris deposits Recent alluvialdeposits Gabbro Terrace deposits Talus deposits
Ursula stock 5°47’30’’N 5°58’30’’N 6°9’30’’N 6°15’0’’N 6°20’30’’N 6°4’0’’N 55’’N7°63’N7°10’ 75°34’30’’N 75°41’0’’N 75°46’30’’N 75°52’0’’N MC 55’’N7°63’N7°10’ 75°34’30’’N 75°41’0’’N 75°46’30’’N 75°52’0’’N AB 06 km Fig. 2Bernetetal. CA
5°53’0’’N 6°4’0’’N 6°9’30’’N 6°15’0’’N 6°20’30’’N 5°58’30’’N 5°47’30’’N
CERRO AMARILLO SECTION
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Scoria Ignimbrite
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Covered with vegetation
JJ001-23 CA-22 JJ001-20 100 JJ001-18 JJ001-17 JJ001-13 CA-18 JJ001-9
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Fig. 3 Bernet et al. ANZA - BOLOMBOLO SECTION
Trachy-andesite and pyroclastic sequence Tuffaceous sequence
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LEGEND LITHOLOGY
Pyroclastic breccia Tuff Lapilli tuff and agglomerate Fig. 4 Bernet et al.
Pyroclastic Undiferentiated Trachy- flow lava flow andesite CONTACTS
Abrupt Erosional
Gradational LA METIDA CREEK SECTION
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QLM -1 Lapilli tuff Pyroclastic breccia flow QLM -6 QLM -7 Tuffaceous Volcaniclastic sandstone sandstone STRUCTURES QLM -9 Ripples Cross- Load structures 40 bedding QLM -10 Lenses Nodules Bio- turbation
Organic Fossils matter
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Fig. 5 Bernet et al. ŽŵďŝĂ&ŽƌŵĂƟŽŶĐŽŵďŝŶĞĚ&dĚĂƚĂ;ŶсϯϬϮͿ ŽŵďŝĂ&ŽƌŵĂƟŽŶĐŽŵďŝŶĞĚ&dĚĂƚĂ;ŶсϯϰϲͿ Central age = 8.54 ± 0.66 Ma (1 ʍͿ Central age = 9.1 ± 0.24 Ma (1ʍͿ 79Ma Dispersion = 34 % Dispersion = 52 % 319Ma 60 250 P(ʖϸͿсϬ͘ϬϬ 50 P(ʖϸͿсϬ͘ϬϬ 200 40 150 30 100 20
50 2 10 0 -2
2 0 -2
0.99Ma 0.7Ma
Ns+Ni 0 4 16 36 64 100 144 196 Ns+Ni 0 12 49 110 196 306 441
77.00U [ppm] 1590.00
Fig 6 Bernet et al. A) Quartz
Lava flows Cerro Amarillo Anzá – Bolombolo
Quartz andesite
Rhyolite Dacite
Alkali rhyolite Rhyodacite
Quartz Andesite Andesite, Quartz Quartz latite alkali Quartz latite quartz- basalt trachyte andesite/basalt trachyte basalt Alkali trachyte Trachyte Latite Latite andesite/basalt Alkali -feldspar Plagioclase
B) Glass
Pyroclastic rocks La Metida Creek section Anzá – Bolombolo section
Vitric tuff
Lithic tuff Crystal tuff
Rock fragments Crystals
Fig 7 Bernet et al. 12 - 6 Ma magmatism A) F F F Marriner & Millward (1984)
Ordoñez (2001)
A = Na2O + K2O Leal-Mejia (2011) Tholeiitic F = FeO Tholeiitic M = MgO Tholeiitic
Calc-alkaline
A M Calc-alkaline Calc-alkaline
Cerro Amarillo Anzá – Bolombolo A AM
B) 18 Ultrabasic Basic Intermediate Acid 12-6 Ma Marriner & Millward (1984) alkaline 12-6 Ma Ordoñez (2001) 17-9 Ma Leal-Mejia (2011) 15 24-20 Ma Leal-Mejia (2011)
Phonolite 12 P-N Trachyte
P-T Benmorite O (wt%)
2 9 Trachy Rhyolite Mugearite andesite B+T O+K Hawaiite 2 6 Nephelin Dacite Na
Andesite 3 Basalt B-A Anzá – Bolombolo Cerro Amarillo 0 35 45 55 65 75 SiO2 (wt%)
Fig. 8 Bernet et al. A) B)
1000 100 Trace elements Cerro Amarillo Rare Earth Elements Cerro Amarillo Anzá – Bolombolo Anzá – Bolombolo 100
10
10 Sample/REEchondrite Sample/Primitive mantle Sample/Primitive Combia Fm (this study) Combia Fm (this study) normalized to primordial mantle after McDonough and Sun (1995) normalized to chondrite after Evensen et al. (1978) 1 1 Cs RbBa Th U Nb Ta La Ce Pr PbNd Sr Sm Zr Hf Eu Gd Tb DyHo Y Er Li Yb Lu La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu
C) 1000 D) 1000 17–6 Ma hypabyssal porphyritic rocks 17–6 Ma hypabyssal porphyriticrocks 12–6 Ma Combia Fm. 12–6 Ma Combia Fm. 100 3–0 Ma volcanicm 100
10
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1 Sample/REEchondrite Sample/Primitive mantle Sample/Primitive Data from Leal-Mejia (2011) Data from Leal-Mejia (2011) normalized to chondrite after Sun and McDonough (1989) normalized to primordial mantle after Wood et al. (1979) 1
Cs Rb Ba Th UKNdTa Nb La CeSr P HfZr Sm Ti Tb Y La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu
E) 1400
1200
1000 Slab
800 dehydration
Ba/Th 600
400 Cerro Amarillo Sediment 200 Anzá – Bolombolo melting 0 024681012 La/Sm
Fig. 9 Bernet et al. A) B) 1000 800 900 Addition of 700 effect of slab 800 aqueous dehydration 600 700 fluids to the magma eastern Amagá basin 600 500 500 400 Sr/Th 400 Ba/Th 300 western Amagá basin 300 Anzá – Bolombolo 200 200 Cerro Amarillo 100 Anzá – Bolombolo 100 Altered Oceanic Crust Cerro Amarillo 0 0 0.702 0.704 0.706 0.708 0.710 0.712 0.5118 0.5120 0.5122 0.5124 0.5126 0.5128 0.5130 0.5132 87Sr/86Sr 143Nd/144Nd C) MORB 0.5130 Northern Anzá – Bolombolo Volcanic Cerro Amarillo Zone 0.5128 Southern
Nd Volcanic
144 0.5126 Zone
Nd/ Compilation of typical
143 Andean volcanism 0.5124 isotopic compositions from Marin-Ceron et al. (2019)
0.5122 Central Volcanic Zone
0.5120 0.702 0.705 0.710 0.715 87Sr/86Sr
Fig 10 Bernet et al. 39.4 A) Paleozoic Precambrian basement 39.0 basement CVZ NVZ 38.6 CVZ Pb SVZ Galapagos Cretaceous 204 38.2 Pacific metaliferous and AOC basement Pb/ carbonate-rich sediments ODP hole & LCC 208 37.8 504B xenolith NVZ Present-day Andean volcanism 37.4 NVZ = Northern volcanic zone Anzá – Bolombolo CVZ = Central volcanic zone Cerro Amarillo SVZ = Southern volcanic zone 37.0 17.0 17.2 17.4 17.6 17.8 18.0 18.2 18.4 18.2 18.8 19.0 19.2 19.4 B) 206Pb/204Pb
39.0 Lower Hemipelagic Andean Continental sediments Paleozoic Crust basement 38.6
Pb ODP hole Paficic 504B
204 sediments Carbonaceous 38.2 Altered
Pb/ sediments oceanic crust 208
37.8 Mantle wedge Squares present possible end-members Anzá – Bolombolo Cerro Amarillo 37.4 18.2 18.4 18.6 18.8 19.0 19.2 19.4 206Pb/204Pb
Fig. 11 Bernet et al. Western Eastern Amagá basin Amagá basin boundary boundary
Anzá – Bolombolo Cerro Amarillo La Metida Creek Upper Continental Crust Lower Continental Crust
Mantle wedge Magmatic processes (AFC & MASH)
Subduction HS+CS Primary components AOC magma Sediment melting, dehydration/ decarbonation
Fig. 12 Bernet al.